Dataset Viewer
Auto-converted to Parquet Duplicate
Search is not available for this dataset
image
imagewidth (px)
256
256
label
class label
0 classes
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
null
End of preview. Expand in Data Studio

LB-DLPU: An L-Band (NISAR/UAVSAR) Benchmark for InSAR Phase Unwrapping

LB-DLPU: example wrapped phase (input) and ground-truth unwrapped phase (target) across regimes and difficulty strata

LB-DLPU is a physically-simulated benchmark for interferometric SAR (InSAR) phase unwrapping at L-band, calibrated to the NISAR (spaceborne, 20 m) and UAVSAR (airborne, 6 m) regimes. Each of the 10,000 patches ships with the wrapped phase, the ground-truth absolute phase, coherence, per-edge integer ambiguity labels, residues, and a validity mask — everything needed to train, validate, and test learning-based and classical unwrappers.

Two properties set it apart from existing (C-band, RMSE-only) PU datasets:

  • Well-posedness certificate. Every scene is provably recoverable: a noiseless-oracle minimum-cost-flow (MCF) unwrapper reconstructs each patch to within 0.035 rad given the correct per-edge costs (100% of 10,000 scenes pass; max clean-oracle RMSE = 0.0347 rad). Any error a method incurs is attributable to the method, not to an unsolvable target.
  • L-band-specific difficulty. Calibrated coherence (Beta fits to real granules), Cramér–Rao phase noise, an ionospheric screen (NISAR), and steep near-fault gradients that push the true per-edge ambiguity into the five-arc range {−2,…,+2}.

Dataset at a glance

Patches 10,000 (256 × 256)
Splits train 8,000 / val 1,000 / test 1,000
Regimes NISAR (20 m, ionosphere on), UAVSAR (6 m, ionosphere off)
Difficulty strata smooth (3,090) / mixed (4,015) / dense (2,895)
Labels absolute phase, per-edge ambiguity (kx, ky), residues
Quicklooks wrapped-phase PNG per patch
Topography 29 Copernicus GLO-30 DEM tiles, whole-tile split (no terrain leakage)

Per-regime statistics (from datasheet.md):

sensor n mean coherence posting residues/Mpix (sim) residues/Mpix (real)
nisar 5,940 0.57 20 m 19,535 18,100
uavsar 4,060 0.40 6 m 33,948 28,794

Directory layout

LB_DLPU/
├── README.md              # this card
├── datasheet.md           # auto-generated statistics + well-posedness certificate
├── dem_manifest.csv       # DEM tile → split assignment (tile, split, region, regime)
├── index.jsonl            # one JSON record per patch (metadata, no arrays)
├── assets/                # figures used in this card
│   ├── preview.png
│   └── dem_tiles_map.png
├── sim/
│   ├── train/  000000.h5 … 007999.h5      (8,000)
│   ├── val/    008000.h5 … 008999.h5      (1,000)
│   └── test/   009000.h5 … 009999.h5      (1,000)
└── sim_wrapped_png/       # wrapped-phase quicklooks, mirroring sim/
    ├── train/  000000.png … 007999.png
    ├── val/    008000.png …
    └── test/   009000.png …

Patch ids are shared across sim/<split>/<id>.h5 and sim_wrapped_png/<split>/<id>.png.

Per-patch HDF5 schema

Each .h5 file (≈0.7 MB) contains:

dataset shape dtype description
psi (256, 256) float32 wrapped phase (network input), radians in (−π, π]; noisy
phi (256, 256) float32 ground-truth absolute (unwrapped) phase, radians
coherence (256, 256) float32 interferometric coherence, [0, 1]
kx (256, 255) int8 horizontal per-edge integer ambiguity, {−2,…,+2}
ky (255, 256) int8 vertical per-edge integer ambiguity, {−2,…,+2}
residues (255, 255) int8 Goldstein loop residues of psi, {−1, 0, +1}
water_mask (256, 256) bool invalid / no-signal pixels (excluded from metrics)

psi is the noisy wrapped observation and phi the clean target; they are not exactly congruent (that is the noise the unwrapper must survive). The per-edge labels satisfy Δφ_e = W(Δψ)_e + 2π·k_e, where W wraps to (−π, π].

Per-patch attributes (HDF5 .attrs): sensor (nisar|uavsar), difficulty (smooth|mixed|dense), mean_coherence, px_m (pixel spacing), NL (looks), residue_count, residues_per_mp, max_grad_rad_per_px, frac_edges_k1, frac_edges_k2, label_clip_frac, water_frac, clean_oracle_rmse, seed, and components (JSON: topography / deformation / atmosphere / ionosphere provenance).

index.jsonl

One record per patch with the same metadata as the HDF5 attributes plus id and split, for fast filtering without opening every file:

{"id": "000000", "split": "train", "sensor": "nisar", "difficulty": "smooth",
 "mean_coherence": 0.56, "NL": 8, "px_m": 20.0, "residue_count": 2182,
 "residues_per_mp": 33294.7, "clean_oracle_rmse": 0.0, "seed": 939529293,
 "components": {"topo_src": "dem", "topo": {"B_perp_m": 32.97}, ...}}

Splits

Train / val / test are disjoint by whole DEM tile: the 29 Copernicus GLO-30 tiles (worldwide tectonic, volcanic, and glacial terrain) are partitioned 17 / 5 / 7, so no terrain is shared across splits and the test set measures generalization to unseen geography. The exact tile → split assignment is in dem_manifest.csv.

Global distribution of the 29 GLO-30 DEM tiles, colored by split (17 train / 5 validation / 7 test)

Loading

import h5py, glob

def load_patch(path):
    with h5py.File(path, "r") as f:
        return {k: f[k][:] for k in f}, dict(f.attrs)

for p in sorted(glob.glob("sim/test/*.h5"))[:1]:
    arrays, attrs = load_patch(p)
    psi, phi = arrays["psi"], arrays["phi"]          # input, target
    print(attrs["sensor"], attrs["difficulty"], psi.shape)

Quicklooks are plain PNGs:

from PIL import Image
Image.open("sim_wrapped_png/test/009000.png")        # wrapped-phase preview

Intended use

Training and benchmarking L-band phase-unwrapping methods — deep networks (wrap-count regression/classification, gradient estimation) and classical / minimum-cost-flow solvers — with per-regime × difficulty evaluation. The well-posedness certificate makes the test split a fair ceiling reference; the per-edge labels support both pixel-wise and edge-wise supervision.

Reference baselines

A method-blind evaluation harness scores every unwrapper on the identical test split, per regime × difficulty, on RMSE, MAE, PSNR, SSIM, a cycle-slip (jump) rate, residue count, and five-arc |k|≥2 edge accuracy. Reference findings across classical, minimum-cost-flow, and in-domain-trained deep baselines:

  • Deep networks train cleanly on this data and outperform classical and statistical solvers (e.g. SNAPHU) — especially on the dense/high-gradient stratum, which the benchmark is designed to stress.
  • The minimum-cost-flow family is residue-free by construction; with the correct per-edge costs the certified oracle ceiling reaches near-zero, residue-free error, while gradient-domain methods leave residues.
  • The benchmark is not saturated: a gap to the oracle ceiling remains for every deployable method, and the strata form a genuine difficulty gradient (error widens smooth → mixed → dense).

The full leaderboard, metric definitions, and significance tests are in the accompanying code/paper.

Limitations and considerations

  • Synthetic ground truth. phi is physically modelled (topography from real Copernicus DEMs; coherence, noise, and ionosphere calibrated to real NISAR / UAVSAR granules) but is not field-validated absolute truth. It is intended for supervised training and controlled benchmarking; real-scene generalization should be assessed separately.
  • Two regimes. Sensor characteristics are approximated for NISAR-like and UAVSAR-like acquisitions; other L-band sensors may differ.
  • No decorrelation-only patches. Every scene is certified recoverable given correct costs; the benchmark isolates cost/prior estimation, not irrecoverable-noise regimes.

Provenance and licensing

  • Topography: Copernicus GLO-30 DEM (© ESA / Copernicus; free and open, attribution required).
  • Noise / coherence / ionosphere models: calibrated to real NISAR L2 GUNW and UAVSAR granules.
  • Simulated phase, labels, and quicklooks: this release.

License: CC-BY-4.0. Free to use, share, and adapt with attribution. The Copernicus GLO-30 DEM attribution above must be retained. If you intend a different license, update both this line and the license: field in the card metadata before publishing.

Citation

If you use LB-DLPU, please cite both the dataset and the accompanying paper.

Dataset (Zenodo):

@dataset{dagbanja_lbdlpu_data_2026,
  title     = {LB-DLPU: An L-Band (NISAR/UAVSAR) Benchmark for InSAR Phase Unwrapping},
  author    = {Dagbanja, S. and Qian, J.},
  year      = {2026},
  publisher = {Zenodo},
  doi       = {10.5281/zenodo.21768604},
  url       = {https://huggingface.co/datasets/TheDagbanja/L-Band_DLPU}
}

Paper:

@article{dagbanja_lbdlpu_paper_2026,
  title   = {LB-DLPU: A Well-Posedness-Certified, NISAR/UAVSAR-Calibrated L-Band Benchmark for InSAR Phase Unwrapping},
  author  = {Dagbanja, S., Qian, J. and Haitao, L.},
  journal = {#Will be updated upon publication},
  year    = {2026},
  note    = {under review}
}
Downloads last month
305